Understanding the orbital period and accretion torque in the ultra-luminous X-ray pulsar NGC 7793 P13 (2019)
Attributed to:
Supermassive black hole growth - a small-scale solution to a large-scale problem
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Type: Working Paper
Volume: 17
Parent Publication: AAS/High Energy Astrophysics Division